Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phys...37...57k&link_type=abstract
Physica Scripta (ISSN 0031-8949), vol. 37, no. 1, Jan. 1988, p. 57-61. SERC-supported research.
Astronomy and Astrophysics
Astrophysics
18
Atomic Excitations, Beryllium, Electron Impact, Electron Transitions, Electron Orbitals, Interpretation, Reaction Kinetics
Scientific paper
The R-matrix electron excitation rates determined by Berrington et al. (1985) for C III, O V, Ne VII, and Si XI and by Dufton et al. (1983) for Ca XVII are used to interpolate the rates for Be-like P XII, S XIII, Cl XIV, Ar XV, and K XVI. The results are presented in a series of tables and briefly characterized. The accuracy of the present findings is estimated as + or - 10 percent within 0.8 dex of log Tmax, where Tmax is the temperature of maximum fractional abundance for ionization equilibrium. The applicability of the results to the diagnostics of astrophysical and laboratory plasmas is indicated.
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